Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:1510.06960.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T12:59:20.293585Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-02T06:26:43.465960Z
Reference resolution
0 of 0 outbound references displayed
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External citation measurements
No source-named external measurement is stored.
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 8b54e886-749b-4eab-9c24-01c5b0f628f9 · inbound
Asteroseismology of solar-type stars cites this paper.
Asteroseismology of solar-type stars Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars
Reference 174
- Resolution
- verified exact
- local_arxiv, observed 2026-05-25T14:15:54.710051Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation f199d942-ddcd-4895-a557-33d8cf151312 · inbound
Asteroseismology cites this paper.
Asteroseismology Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars
Reference 10
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T20:13:24.414392Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 22d982f0-5348-44e4-98c2-f6bc71674829 · inbound
Seismic signature of a magnetic field in the $\gamma$ Doradus star KIC 2309579 cites this paper.
Seismic signature of a magnetic field in the $\gamma$ Doradus star KIC 2309579 Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars
Reference 8
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-22T03:54:33.828049Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation e5ccd01d-f0d2-458e-8890-0ed99074f751 · inbound
Non-linear Dynamical Stability of Magnetic Polytropes cites this paper.
Non-linear Dynamical Stability of Magnetic Polytropes Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars
Reference 28
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T18:52:30.557008Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation ed39607c-6e07-4c54-8dbd-3ef761a00935 · inbound
Extending asteroseismic magnetometry across the diverse landscape of magnetic structures cites this paper.
Extending asteroseismic magnetometry across the diverse landscape of magnetic structures Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars
Reference 10
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-27T20:41:14.469842Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation c2c6080a-a355-4784-ad33-1de9a9b416a3 · inbound
Oscillations of red giant stars with magnetic damping in the core. II. Mixed mode visibilities on the red-giant branch cites this paper.
Oscillations of red giant stars with magnetic damping in the core. II. Mixed mode visibilities on the red-giant branch Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars
Reference 124
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T03:31:30.822544Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation bae1a321-56f7-43b0-99b6-8a8223738ef0 · inbound
The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors cites this paper.
The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars
Reference 104
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-27T05:40:36.413143Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation a03d8e34-4396-4146-a536-ce348aba4e87 · inbound
Constraining the model-based uncertainties of asteroseismic magnetic field measurements in red giants cites this paper.
Constraining the model-based uncertainties of asteroseismic magnetic field measurements in red giants Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars
Reference 73
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-02T06:26:43.467164Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation f9a16161-fe92-41c0-abc8-b88a3a1e3b0b · inbound
Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations cites this paper.
Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars
Reference 41
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T12:59:20.293585Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.